Information Loss in Black Hole Evaporation
arXiv:hep-th/0512121 · doi:10.1142/S0217732306019980
Abstract
Parikh-Wilczek tunnelling framework is investigated again. We argue that Parikh-Wilczek's treatment, which satisfies the first law of black hole thermodynamics and consists with an underlying unitary theory, is only suitable for a reversible process. Because of the negative heat capacity, an evaporating black hole is a highly unstable system. That is, the factual emission process is irreversible, the unitary theory will not be satisfied and the information loss is possible.
4 pages, RevTex; added references
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